1,009 research outputs found

    Interference Effects in the Decays of Spin-Zero Resonances into γγ\gamma \gamma and ttˉt\bar{t}

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    We consider interference effects in the production via gluon fusion in LHC collisions at 13 TeV and decays into γγ\gamma \gamma and ttˉt {\bar t} final states of one or two putative new resonant states Φ\Phi, assumed here to be scalar and/or pseudo scalar particles. Although our approach is general, we use for our numerical analysis the example of the putative 750750 GeV state for which a slight excess was observed in the initial LHC 1313 TeV data. We revisit previous calculations of the interferences between the heavy-fermion loop-induced ggΦγγgg \to \Phi \to \gamma \gamma signal and the continuum ggγγgg\to \gamma\gamma QCD background, which can alter the production rate as well as modify the line-shape and apparent mass. We find a modest enhancement by 20\sim 20% under favorable circumstances, for a large Φ\Phi width. The effect of interference on the apparent scalar-pseudoscalar mass difference in a two-Higgs-doublet model is found to be also modest. An exploratory study indicates that similar effects are to be expected in the ggΦZγgg \to \Phi \to Z \gamma channel. In this and other models with a large Φ\Phi total width, the dominant Φ\Phi decays are expected to be into ttˉt \bar t final states. We therefore also study the effects of interference of the ggΦttˉgg\to \Phi \to t\bar t signal with the ggttˉgg\to t \bar t continuum QCD background and show that in the presence of standard fermions only in the ggΦgg\to \Phi loops, it is destructive causing a dip in the ttˉt \bar t mass distribution. Including additional vector-like quarks leads to a different picture as peaks followed by dips can then occur. We use the absence of such effects in ATLAS and CMS data to constrain models of the production and decays of the Φ\Phi state(s).Comment: 31 pages, v2 contains additional comment

    Prospects for Higgs physics at energies up to 100 TeV

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    We summarise the prospects for Higgs boson physics at future proton-proton colliders with centre of mass (c.m.) energies up to 100 TeV. We first provide the production cross sections for the Higgs boson of the Standard Model from 13 TeV to 100 TeV, in the main production mechanisms and in subleading but important ones such as double Higgs production, triple production and associated production with two gauge bosons or with a single top quark. We then discuss the production of Higgs particles in beyond the Standard Model scenarios, starting with the one in the continuum of a pair of scalar, fermionic and vector dark matter particles in Higgs-portal models in various channels with virtual Higgs exchange. The cross sections for the production of the heavier CP-even and CP-odd neutral Higgs states and the charged Higgs states in two-Higgs doublet models, with a specific study of the case of the Minimal Supersymmetric Standard Model, are then given. The sensitivity of a 100 TeV proton machine to probe the new Higgs states is discussed and compared to that of the LHC with a c.m. energy of 14 TeV and at high luminosity.Comment: 61 pages, 16 figures, 6 tables; review article. v2: numbers and figures updated, aknowledgments modified, references added and typos corrected. Matches the published versio

    Future Collider Signatures of the Possible 750 GeV State

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    If the recent indications of a possible state Φ\Phi with mass 750\sim 750 GeV decaying into two photons reported by ATLAS and CMS in LHC collisions at 13 TeV were to become confirmed, the prospects for future collider physics at the LHC and beyond would be affected radically, as we explore in this paper. Even minimal scenarios for the Φ\Phi resonance and its γγ\gamma \gamma decays require additional particles with masses 12mΦ\gtrsim \frac12 m_\Phi. We consider here two benchmark scenarios that exemplify the range of possibilities: one in which Φ\Phi is a singlet scalar or pseudoscalar boson whose production and γγ\gamma \gamma decays are due to loops of coloured and charged fermions, and another benchmark scenario in which Φ\Phi is a superposition of (nearly) degenerate CP-even and CP-odd Higgs bosons in a (possibly supersymmetric) two-Higgs doublet model also with additional fermions to account for the γγ\gamma \gamma decay rate. We explore the implications of these benchmark scenarios for the production of Φ\Phi and its new partners at colliders in future runs of the LHC and beyond, at higher-energy pppp colliders and at e+ee^+ e^- and γγ\gamma \gamma colliders, with emphasis on the bosonic partners expected in the doublet scenario and the fermionic partners expected in both scenarios.Comment: 52 pages, 24 figures, v2 corrects two plots and some typos, and contains a new section on production in electron-positron collisions as well as additional reference

    Thermal and non-thermal production of dark matter via Z'-portal(s)

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    We study the genesis of dark matter in the primordial Universe for representative classes of Z'-portals models. For weak-scale Z' mediators we compute the range of values of the kinetic mixing allowed by WMAP/PLANCK experiments corresponding to a FIMP regime. We show that very small values of the kinetic coupling (1.e-12 < delta < 1.e-11) are sufficient to produce the right amount of dark matter. We also analyse the case of very massive gauge mediators, whose mass is larger than the reheating temperature, "T_RH", with a weak-scale coupling to ordinary matter. Relic abundance constraints then impose a direct correlation between T_RH and the effective scale "Lambda" of the interactions: Lambda ~ 1.e3--1.e5 * T_RH. Finally we describe in some detail the process of dark thermalisation and study its consequences on the computation of the relic abundance.Comment: version accepted for publication in JCA

    Searching for the QCD Axion with Gravitational Microlensing

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    The phase transition responsible for axion dark matter production can create large amplitude isocurvature perturbations which collapse into dense objects known as axion miniclusters. We use microlensing data from the EROS survey, and from recent observations with the Subaru Hyper Suprime Cam to place constraints on the minicluster scenario. We compute the microlensing event rate for miniclusters treating them as spatially extended objects with an extended mass function. Using the published bounds on the number of microlensing events we bound the fraction of DM collapsed into miniclusters, fMCf_{\rm MC}. For an axion with temperature dependent mass consistent with the QCD axion we find fMC<0.22(ma/100μeV)0.57f_{\rm MC}<0.22(m_a/100\,\mu\text{eV})^{-0.57}, which represents the first observational constraint on the minicluster fraction. We forecast that a high-efficiency observation of ten nights with Subaru would be sufficient to constrain fMC0.1f_{\rm MC}\lesssim 0.1 over the entire QCD axion mass range. We make various approximations to derive these constraints and dedicated analyses by the observing teams of EROS and Subaru are necessary to confirm our results. If accurate theoretical predictions for fMCf_{\rm MC} can be made in future then microlensing can be used to exclude, or discover, the QCD axion. Further details of our computations are presented in a companion paper.Comment: 5 pages, 4 figures, v2 contains an improved description of our modeling of miniclusters and lensing with revised limits, matches version accepted in PR

    Fully covering the MSSM Higgs sector at the LHC

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    In the context of the Minimal Supersymmetric extension of the Standard Model (MSSM), we reanalyze the search for the heavier CP-even HH and CP-odd AA neutral Higgs bosons at the LHC in their production in the gluon-fusion mechanism and their decays into gauge and lighter hh bosons and into top quark pairs. We show that only when considering these processes, that one can fully cover the entire parameter space of the Higgs sector of the model. Indeed, they are sensitive to the low tanβ\tan\beta and high Higgs mass ranges, complementing the traditional searches for high mass resonances decaying into τ\tau-lepton pairs which are instead sensitive to the large and moderate tanβ\tan\beta regions. The complementarity of the various channels in the probing of the complete [tanβ,MA][\tan\beta, M_A] MSSM parameter space at the previous and upcoming phases of the LHC is illustrated in a recently proposed simple and model independent approach for the Higgs sector, the hhMSSM, that we also refine in this paper.Comment: 44 pages, 21 figures, pdflate

    Mixed Heavy-Light Matching in the Universal One-Loop Effective Action

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    Recently, a general result for evaluating the path integral at one loop was obtained in the form of the Universal One-Loop Effective Action. It may be used to derive effective field theory operators of dimensions up to six, by evaluating the traces of matrices in this expression, with the mass-dependence encapsulated in the universal coefficients. Here we show that it can account for loops of mixed heavy-light particles in the matching procedure. Our prescription for computing these mixed contributions to the Wilson coefficients is conceptually simple. Moreover it has the advantage of maintaining the universal structure of the effective action, which we illustrate using the example of integrating out a heavy electroweak triplet scalar coupling to a light Higgs doublet. Finally we also identify new structures that were previously neglected in the universal results.Comment: 22 pages, 3 figures; v2: expanded discussion in Section 3, typos correcte

    Extending the Universal One-Loop Effective Action: Heavy-Light Coefficients

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    The Universal One-Loop Effective Action (UOLEA) is a general expression for the effective action obtained by evaluating in a model-independent way the one-loop expansion of a functional path integral. It can be used to match UV theories to their low-energy EFTs more efficiently by avoiding redundant steps in the application of functional methods, simplifying the process of obtaining Wilson coefficients of operators up to dimension six. In addition to loops involving only heavy fields, matching may require the inclusion of loops containing both heavy and light particles. Here we use the recently-developed covariant diagram technique to extend the UOLEA to include heavy-light terms which retain the same universal structure as the previously-derived heavy-only terms. As an example of its application, we integrate out a heavy singlet scalar with a linear coupling to a light doublet Higgs. The extension presented here is a first step towards completing the UOLEA to incorporate all possible structures encountered in a covariant derivative expansion of the one-loop path integral.Comment: 20 pages, 1 figure, 5 tables, 1 Mathematica Noteboo

    Gauge Coupling Unification and Non-Equilibrium Thermal Dark Matter

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    We study a new mechanism for the production of dark matter in the universe which does not rely on thermal equilibrium. Dark matter is populated from the thermal bath subsequent to inflationary reheating via a massive mediator whose mass is above the reheating scale, T_R. To this end, we consider models with an extra U(1) gauge symmetry broken at some intermediate scale M, of the order of 10^10 -- 10^12 GeV. We show that not only does the model allow for gauge coupling unification (at a higher scale associated with grand unification) but can naturally provide a dark matter candidate which is a Standard Model singlet but charged under the extra U(1). The intermediate scale gauge boson(s) which are predicted in several E6/SO(10) constructions can be a natural mediator between dark matter and the thermal bath. We show that the dark matter abundance, while never having achieved thermal equilibrium, is fixed shortly after the reheating epoch by the relation T_R^3/M^4. As a consequence, we show that the unification of gauge couplings which determines M also fixes the reheating temperature T_R, which can be as high as 10^11 GeV.Comment: 4 pages, 2 figures, 1 tabl
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